Bohrium is a
chemical element in the
periodic table that has the symbol
Bh and
atomic number 107.
It is a
synthetic element whose most stable
isotope, Bh-270, has a
half-life of 61
seconds. Chemical experiments confirmed bohrium's predicted position as a member of group 7 of the
periodic table, as a heavier homologue to rhenium.
Official discovery
The first convincing synthesis was in 1981 by a German research team led by
Peter Armbruster and
Gottfried Münzenberg at the
Gesellschaft für Schwerionenforschung (Institute for Heavy Ion Research) in
Darmstadt using the Dubna reaction.
In 1989, the GSI team successfully repeated the reaction during their efforts to measure an excitation function. During these experiments, 261Bh was also identified in the 2n evaporation channel and it was confirmed that 262Bh exists as two isomers.
The IUPAC/IUPAP Transfermium Working Group (TWG) report in 1992 officially recognised the GSI team as discoverers of element 107.
Proposed names
Historically element 107 has been referred to as
eka-rhenium.
The Germans suggested the name nielsbohrium with symbol Ns to honor the Danish physicist Niels Bohr. The Soviets had suggested this name be given to element 105 (dubnium) and the German team wished to recognise both Bohr and the fact that the Dubna team had been the first to propose the cold fusion reaction.
There was an element naming controversy as to what the elements from 101 to 109 were to be called; thus IUPAC adopted unnilseptium (or /ˌʌnɪlˈsɛptiəm/, symbol Uns) as a temporary, systematic element name for this element. In 1994 a committee of IUPAC rejected the name nielsbohrium since there was no precedence for using a scientist's complete name in the naming of an element and thus recommended that element 107 be named bohrium.
This was opposed by the discoverers who were adamant that they had the right to name the element. The matter was handed to the Danish branch of IUPAC who voted in favour of the name bohrium. There was some concern however that the name might be confused with boron and in particular the distinguishing of the names of their respective oxo-ions bohrate and borate. Despite this, the name bohrium for element 107 was recognized internationally in 1997. The IUPAC subsequently decided that bohrium salts should be called bohriates.
Electronic structure
Bohrium is element 107 in the Periodic Table. The two forms of the projected electronic structure are:
Bohr model: 2, 8, 18, 32, 32, 13, 2
Quantum mechanical model: 1s22s22p63s23p64s23d10
4p65s24d105p66s24f145d10
6p67s25f146d5
Extrapolated chemical properties of eka-rhenium/dvi-technetium
Oxidation states
Element 107 is projected to be the fourth member of the 6d series of transition metals and the heaviest member of group VII in the Periodic Table, below
manganese,
technetium and
rhenium.
All the members of the group readily portray their group oxidation state of +VII and the state becomes more stable as the group is descended. Thus bohrium is expected to form a stable +VII state.
Technetium also shows a stable +IV state whilst rhenium portrays stable +IV and +III states. Bohrium may therefore show these lower states as well.
Chemistry
The heavier members of the group are known to form volatile heptoxides M
2O
7, so bohrium should also form the volatile oxide Bh
2O
7. The oxide should dissolve in water to form perbohric acid, HBhO
4.
Rhenium and technetium form a range of oxyhalides from the halogenation of the oxide. The chlorination of the oxide forms the oxychlorides MO
3Cl, so BhO
3Cl should be formed in this reaction. Fluorination results in MO
3F and MO
2F
3 for the heavier elements in addition to the rhenium compounds ReOF
5 and ReF
7. Therefore, oxyfluoride formation for bohrium may help to indicate eka-rhenium properties.
Industrial and commercial use
Like
seaborgium and
hassium, its neighbours, bohrium has no industrial or commercial use due to its extremely short half-life. Few atoms have ever been made, but if enough were found in one area, bohrium would constitute a radiation hazard.
Experimental chemistry
Gas phase chemistry
In 2000, a team at the PSI conducted a chemistry reaction using atoms of
267Bh produced in the reaction between Bk-249 and Ne-22 ions. The resulting atoms were thermalised and reacted with a HCl/O
2 mixture to form a volatile oxychloride. The reaction also produced isotopes of its lighter homologues,
technetium (as
108Tc) and
rhenium (as
169Re). The isothermal adsorption curves were measured and gave strong evidence for the formation of a volatile oxychloride with properties similar to that of rhenium oxychloride. This placed bohrium as a typical member of group 7.
Summary of compounds
| Formula
| Names(s) |
| BhO3Cl
| bohrium oxychloride ; bohrium(VII) chloride trioxide |
History of synthesis of isotopes by cold fusion
209Bi(54Cr,xn)263-xBh (x=1,2)
The synthesis of element 107 was first attempted in 1976 by scientists at the
Joint Institute for Nuclear Research at
Dubna using this cold fusion reaction. Analysis was by detection of
spontaneous fission (SF). They discovered two SF activities, one with a 1-2 ms half-life and one with a 5 s activity. Based on the results of other cold fusion reactions, they concluded that they were due to
261107 and
257105 respectively. However, later evidence gave a much lower SF branching for
261107 reducing convidence in this assignment. The assignment of the element 105 activity was later changed to
258105, presuming that the decay of element 107 was missed. The 2 ms SF activity was assigned to
258Rf resulting from the 33%
EC branch.
The GSI team studied the reaction in 1981 in their discovery experiments. Five atoms of
262Bh were detected using the method of correlation of genetic parent-daughter decays.
In 1987, an internal report from Dubna indicated that the team had been able to detect the
spontaneous fission of
261107 directly.
The GSI team further studied the reaction in 1989 and discovered the new isotope
261Bh during the measurement of the 1n and 2n excitation functions but were unable to detect an SF branching for
261Bh.
They continued their study in 2003 using newly developed bismuth(III) fluoride (BiF
3) targets, used to provide further data on the decay data for
262Bh and the daughter
258Db.
The 1n excitation function was remeasured in 2005 by the team at LBNL after some doubt about the accuracy of previous data. They observed 18 atoms of
262Bh and 3 atoms of
261Bh and confirmed the two isomers of
262Bh.
209Bi(53Cr,xn)262-xBh
The team at Dubna studied this reaction in 1976 in order to assist in their assignments of the SF activities from their experiments with a Cr-54 beam. They were unable to detect any such activity, indicating the formation of different isotopes decaying primarily by alpha decay.
209Bi(52Cr,xn)261-xBh (x=1)
This reaction was studied for the first time in 2007 by the team at LBNL to search for the lightest bohrium isotope
260Bh. The team successfully detected 8 atoms of
260Bh decaying by correlated 10.16 MeV alpha particle emission to
256Db. The alpha decay energy indicates the continued stabilising effect of the N=152 closed shell.
208Pb(55Mn,xn)263-xBh (x=1)
The team at Dubna also studied this reaction in 1976 as part of their newly established cold fusion approach to new elements. As for the reaction using a Bi-209 target, they observed the same SF activities and assigned them to
261107 and
257105. Later evidence indicated that these should be reassigned to
258105 and
258104 (see above).
In 1983, they repeated the experiment using a new technique: measurement of alpha decay from a descendant using chemical separation. The team were able to detect the alpha decay from a descendant of the 1n evaporation channel, providing some evidence for the formation of element 107 nuclei.
This reaction was later studied in detail using modern techniques by the team at LBNL. In 2005 they measured 33 decays of
262Bh and 2 atoms of
261Bh, providing a 1n excitation function and some spectroscopic data of both
262Bh isomers. The 2n excitation function was further studied in a 2006 repeat of the reaction. . The team found that this reaction had a higher 1n cross section than the corresponding reaction with a Bi-209 target, contrary to expectations. Further research is required to understand the reasons.
Synthesis of isotopes by hot fusion
243Am(26Mg,xn)269-xBh (x=3,4,5)
Recently, the team at the Institute of Modern Physics (IMP), Lanzhou, have studied the nuclear reaction between americium-243 and magnesium-26 ions in order to synthesise the new isotope
265Bh
and gather more data on
266Bh. In two series of experiments, the team has measured partial excitation functions of the 3n,4n and 5n evaporation channels.
249Bk(22Ne,xn)271-xBh (x=4,5)
The first attempts to synthesise element 107 by hot fusion pathways were performed in 1979 by the team at Dubna. The reaction was repeated in 1983. In both cases, they were unable to detect and
spontaneous fission from nuclei of element 107.
More recently, hot fusions pathways to bohrium have been re-investigated in order to allow for the synthesis of more long-lived,
neutron rich isotopes to allow a first chemical study of bohrium. In 1999, the team at LBNL announced the discovery of long-lived
267Bh (5 atoms) and
266Bh (1 atom).
In the following year, the same team attempted to confirm the synthesis and decay of
266Bh. However, they were unable to do so and the identification of
266Bh in the first experiment is questionable.
The team at the Paul Scherrer Institute (PSI) in Bern, Switzerland later synthesised 6 atoms of
267Bh in the first definitive study of the chemistry of bohrium (see below).
254Es(16O,xn)270-xBh
As an alternative means of producing long-lived bohrium isotopes suitable for a chemical study, the synthesis of
267Bh and
266Bh were attempted in 1995 by the team at GSI using the highly asymmetric reaction using an einsteinium-254 target. They were unable to detect any product atoms.
Synthesis of isotopes as decay products
Isotopes of bohrium have also been detected in the decay of heavier elements. Observations to date are shown in the table below:
| Evaporation Residue
| Observed Bh isotope |
| 288115
| 272Bh |
| 287115
| 271Bh (missed) |
| 282113
| 270Bh |
| 278113
| 266Bh |
| 272Rg
| 264Bh |
| 266Mt
| 262Bh |
Chronology of isotope discovery
| Isotope
| Year discovered
| discovery reaction |
| 260Bh
| 2007
| 209Bi(52Cr,n) |
| 261Bh
| 1989
| 209Bi(54Cr,2n) |
| 262Bhg,m
| 1981
| 209Bh(54Cr,n) |
| 263Bh
| unknown
| |
| 264Bh
| 1994
| 209Bi(64Ni,n) |
| 265Bh
| 2004
| 243Am(26Mg,4n) |
| 266Bh
| 2004
| 209Bi(70Zn,n) |
| 267Bh
| 2000
| 249Bk(22Ne,5n) |
| 268Bh
| unknown
| |
| 269Bh
| unknown
| |
| 270Bh
| 2006
| 237Np(48Ca,3n) |
| 271Bh
| unknown
| |
| 272Bh
| 2003
| 243Am(48Ca,3n) |
Isomerism in bohrium nuclides
262Bh
The only confirmed example of isomerism in bohrium is for the isotope
262Bh. Direct production populates two states, a ground state and an isomeric state. The ground state is confirmed as decaying by alpha emission with alpha lines at 10.08,9.82 and 9.76 MeV with a revised half life of 84 ms. The excited state decays by alpha emission with lines at 10.37 and 10.24 MeV with a revised half-life of 9.6 ms.
Chemical yields of isotopes
Cold Fusion
The table below provides cross-sections and excitation energies for cold fusion reactions producing bohrium isotopes directly. Data in bold represents maxima derived from excitation function measurements. + represents an observed exit channel.
| Projectile
| Target
| CN
| 1n
| 2n
| 3n |
| 55Mn
| 208Pb
| 263Bh
| 590 pb , 14.1 MeV
| ~35 pb
|
|
| 54Cr
| 209Bi
| 263Bh
| 510 pb , 15.8 MeV
| ~50 pb
|
|
| 52Cr
| 209Bi
| 261Bh
| 59 pb , 15.0 MeV
|
|
|
Hot Fusion
The table below provides cross-sections and excitation energies for hot fusion reactions producing bohrium isotopes directly. Data in bold represents maxima derived from excitation function measurements. + represents an observed exit channel.
| Projectile
| Target
| CN
| 3n
| 4n
| 5n |
| 26Mg
| 243Am
| 271Bh
| +
| +
| + |
| 22Ne
| 249Bk
| 271Bh
|
| ~96 pb
| + |
References
External links